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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4746
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dc.contributor.authorPandey, A. K-
dc.contributor.authorMahra, H. S-
dc.contributor.authorSagar, R-
dc.date.accessioned2009-08-10T14:48:37Z-
dc.date.available2009-08-10T14:48:37Z-
dc.date.issued1991-
dc.identifier.citationJanes, Kenneth. ed., The formation and evolution of star clusters., Proceedings of a Symposium held as part of the 102nd Summer Scientific Meeting of the Astronomical Society of the Pacific in Boston, ASP Conference Series, Vol. 13, Massachusetts, July 14 – 15, 1990, pp. 170 - 172en
dc.identifier.isbn0-937707-32-5-
dc.identifier.urihttp://hdl.handle.net/2248/4746-
dc.description.abstractThe effect of mass segregation on cluster mass functions has been studied and it is found that the slope of the mass function is steeper in the outer parts of open dusters. Since dynamical relaxation time is always larger than the age of the dusters, it is inferred that the observed mass segregation might have taken place at the time of cluster formation.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.ispartofseriesASP Conference Series; Vol. 13-
dc.relation.urihttp://adsabs.harvard.edu/abs/1991ASPC...13..170Pen
dc.rights© Astronomical Society of the Pacificen
dc.subjectEarly Starsen
dc.subjectOpen Clustersen
dc.subjectSpatial Distributionen
dc.subjectStellar Massen
dc.subjectMass Spectraen
dc.subjectMassive Starsen
dc.subjectStar Formationen
dc.titleA study of the spatial variation of mass functions in some young open clustersen
dc.typeArticleen
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